Physics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993geoae..33....1i&link_type=abstract
Geomagnetizm i Aehronomiya, vol. 33, p. 1
Physics
Interplanetary Medium, Solar Flares, Magnetospheric Instability, Magnetic Clouds, Earth Orbits, Heliosphere, Magnetic Storms, Magnetohydrodynamic Turbulence
Scientific paper
A study is made of the MHD structure of interplanetary disturbances that occur far from the streamer but near the earth helioprojection. It is found that flares in a 'weak' field (3-4 micro T) give rise to structures with magnetic clouds, whereas after flares in a 'strong' field (10-14 micro T), the clouds are either absent or are significantly changed, probably due to the screw instability. The disturbances produced by flares in a 'weak' field are characterized by a low velocity, and their travel toward the earth can be estimated from the head shock front and from the cloud boundary and axis.
Ivanov K. G.
Kharshiladze A. F.
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